34069 Lys transport teori og simulation metoder

2016/2017

Kursusinformation
Light transport theory and simulation methods
Engelsk
5
Kandidat
Januar
Campus Lyngby
Lectures, problem solving, laboratory exercises
3-uger
Aftales med underviser
Bedømmelse af opgave(r)/rapport(er)
Individual or group project with oral presentation
Alle hjælpemidler er tilladt
7-trins skala , intern bedømmelse
34020/34031 , 34020/34031 - Can be taken at the same time
Thierry Silvio Claude Soreze , Risø Campus, Bygning 108, Tlf. (+45) 4677 4543 , tsor@fotonik.dtu.dk

34 Institut for Fotonik
I studieplanlæggeren
Dette kursus giver den studerende en mulighed for at lave eller forberede et projekt som kan deltage i DTUs studenterkonference om bæredygtighed, klimateknologi og miljø (GRØN DYST). Se mere på http://www.groendyst.dtu.dk
Overordnede kursusmål
The theory of optics is so rich and complex that many theoretical formalisms have been formulated to describe, analyze, simulate and quantify its physical properties. Among all these formalisms phenomenological approaches like radiometry and radiative transfer, originally stated in the context of astrophysics, are very convenient and widely used to simulate light propagation and light-matter interactions. Phenomenon like scattering of light by a random media or rough surface are well explained by radiative transfer theory, as well as macroscopic light-matter interactions through the concept of bi-scattering-distribution-function (BSDF). In this course, we will give significant theoretical and practical insights of this theory, which is of particular importance of many fields of science and engineering.
Læringsmål
En studerende, der fuldt ud har opfyldt kursets mål, vil kunne:
  • • Analyze and characterize optical properties of materials important for light transport
  • • Model, derive, measure and efficiently utilize bi-scattering-distribution-functions
  • • Manipulate and solve the integral equations governing light transport in both scalar and vector forms
  • • Simulate and model light transport and light-matter interactions for engineering and scientific applications from optical engineering to astrophysics
  • • Predict and solve the (multiple/single) scattering of light by random scatterers, both in volume and surface
  • • Derive mathematical and numerical models for light transport modeling and simulation
  • • Describe and interpret the principles of optical simulation software and raytracing based algorithms
  • • Conduct numerical simulations for solving complex light transport and light matter interaction problems, without directly solving PDEs like Maxwell’s or Wave equations
  • • Derive analytical solutions of Maxwell’s equations
Kursusindhold
The course consists of four parts:

1. Review of theory of optics
2. Radiative transfer equation (RTE): theory and applications
3. Light scattering and bi-directional scattering functions
4. Numerical methods and algorithms for solving the RTE and scattering problems

We will start from reviewing electromagnetic and wave approaches of principles of optics, and related mathematical concepts. This part will also review optical properties of materials; this will be useful for the modelling and simulation of light transport problems.
In a second part of the course, we will depart from Maxwell’s and wave equations to derive the radiative transfer equation, which is based on geometrical optics but can fully embrace waves optics properties like polarization. In this part of the course, we will also discuss integral equations, as the RTE is part of this class of equations; other integral equations that will be discussed include Kirchhoff and Stratton-Chu integrals.
Then equipped with the theoretical foundation of radiative transfer and integral equations we will approach the problem of light scattering and explain it through the RTE formalism. In this part, we will also introduce the concept of bi-scattering-distribution-function (BSDF). Polarization will be also discussed in this section, and we will see how to include it in a ray-based theory through Stokes formalism and vector integral equations. Based on understanding of the theoretical aspects of radiative transfer we will learn to solve integral equations with raytracing and Monte Carlo methods, and present some commercial and open source simulation packages based on these techniques.
Sidst opdateret
19. oktober, 2016